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Fig. 15


Resulting fluxes from the 2BB model fit in the high temperature epoch 5, plotted over wavelength. Overplotted are our derived NIR and MIR fluxes (zYJHK and W1, W2, W3). While matching the observed HK fluxes better than the 1BB model, the 2BB model total fluxes by far exceed the WISE W1, W2 measurements. A second blackbody component inside of 100 days can be clearly rejected. Again, the model was only fit to our zYJHK data (marked with green circles, while the other data are represented by triangles).

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